1975
DOI: 10.1021/ja00844a007
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Chemical evolution. XXVI. Photochemistry of methane, nitrogen, and water mixtures as a model for the atmosphere of the primitive earth

Abstract: Methane-water vapor mixtures were irradiated using a low pressure mercury lamp and the reaction products were determined at intervals between 0.5 and 6 hr. Formaldehyde, acetaldehyde, and methanol were observed after 0.5 hr. The presence of ethylene glycol, ethanol, acetone, isopropyl alcohol, tert-butyl alcohol, methyl ethyl ketone, isobutyl alcohol, rert-amyl alcohol, and neopentyl alcohol was detected in small amounts after 2 hr and the yields increased after 4 and 6 hr irradiation times. Virtually the same… Show more

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Cited by 57 publications
(28 citation statements)
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“…Two such high-temperature planetary sources are lightning and impacts, which have been contemplated as energy sources for prebiotic molecular synthesis (Chyba & Sagan 1992;Nava-Sedeño et al 2016). However, these sources face the problem of abundance: lightning and impact-driven shockwaves are estimated to have delivered three orders of magnitude less energy than UV photons ( 300 nm < ) to the young Earth (Ferris & Chen 1975). Hence, it is difficult to avoid the conclusion that a paucity of UV light might pose a problem for abiogenesis scenarios on M-dwarf planets like Proxima Centauri b, LHS 1140b, or the TRAPPIST-1 planets.…”
Section: Low-uv On M Dwarfs: a Challenge For Abiogenesis?mentioning
confidence: 99%
“…Two such high-temperature planetary sources are lightning and impacts, which have been contemplated as energy sources for prebiotic molecular synthesis (Chyba & Sagan 1992;Nava-Sedeño et al 2016). However, these sources face the problem of abundance: lightning and impact-driven shockwaves are estimated to have delivered three orders of magnitude less energy than UV photons ( 300 nm < ) to the young Earth (Ferris & Chen 1975). Hence, it is difficult to avoid the conclusion that a paucity of UV light might pose a problem for abiogenesis scenarios on M-dwarf planets like Proxima Centauri b, LHS 1140b, or the TRAPPIST-1 planets.…”
Section: Low-uv On M Dwarfs: a Challenge For Abiogenesis?mentioning
confidence: 99%
“…Interestingly, when other workers in the 1970s and early 1980s attempted to repeat the results of Dodonova (1966) but failed to produce nitriles or N-containing organics in the UV (Ferris and Chen, 1975;Chang et al, 1979;Bossard et al, 1982;Raulin et al, 1982), Bossard et al (1982) concluded that ''UV light is not able to produce nitriles from CH 4 -N 2 mixtures'' and ''UV light is not an efficient source for producing unsaturated carbon chains.'' The results presented herein clearly contradict those conclusions.…”
Section: Trainer Et Almentioning
confidence: 99%
“…Fe 2 + in a cyclotron yields traces of CH20 and formic acid (Garrison et al, 1951). CH20 and higher aldehydes are also formed by the photolysis of H20 in the presence of C~ (Ferris and Chen, 1975b;Bar-Nun and Chang, 1983), the photolysis of CO-H20 mixtures (park and Getoff, 1988) and the photolysis of methanol (Allamandola et al, 1988). It has been tentatively identified as a product of the photolysis of ferrous carbonate (Joe et al, 1986) and~-irradiation of calcium carbonate (Albarran et al, 1987).…”
Section: Formaldehyde and Other Aldehydesmentioning
confidence: 99%